HD 21749
{{Short description|Star in the constellation Reticulum}}
{{use dmy dates|date=January 2019}}
{{starbox begin
|name = HD 21749
}}
{{starbox image
|image = 250px
|caption = HD 21749 – star in the constellation Reticulum
|credit =
}}
{{Starbox observe
| epoch = J2000
| constell = Reticulum
}}
{{Starbox character
| r-i =
| v-r =
| j-h =
| j-k =
| variable =
}}
{{Starbox astrometry
| radial_v ={{val|59.32|0.12}}
| parallax = 61.2271
| p_error = 0.0150
}}
{{Starbox detail
| mass = {{val|0.73|0.07}}
| radius = {{val|0.695|0.030}}
| luminosity = {{val|0.20597|0.00016}}
| gravity = {{val|4.613|0.052|0.061}}
| temperature = {{val|4640|100}}
| metal_fe = {{val|0.003|0.060}}
| rotation = {{val|34.1|2.4|2.7}} d
| rotational_velocity =1.04
| age_gyr = {{val|3.8|3.7}}
}}
{{Starbox catalog
| names = {{odlist|HIP=16069|2MASS=J03265922-6329569|CD=-63 110|CPD=-63 232A|GJ=143|SAO=248808|TYC=8870-01392-1|WDS=J03270-6330A}}, TOI-186
}}
{{Starbox reference
| Simbad = HD+21749
| EPE = HD 21749
}}
{{starbox end}}
HD 21749 is an orange main-sequence star in the constellation Reticulum. It has an apparent visual magnitude of 8.143, which means it is too dim to be seen with the naked eye. From parallax measurements by the Gaia spacecraft, it is located {{convert|53|ly|pc|abbr=on}} from Earth.
In 2019, it was discovered that the star has two exoplanets: a possibly rocky, hot sub-Neptune-sized exoplanet named HD 21749 b; and an Earth-sized exoplanet named HD 21749 c. These exoplanets were discovered by the TESS spacecraft.
Stellar characteristics
HD 21749 is a K-type main sequence star (orange dwarf) with a spectral type of K4.5V, indicating it is smaller and cooler than the Sun. It is estimated to have a mass of {{solar mass|0.73|link=y}}, a radius of {{solar radius|0.70|link=y}}, and a luminosity of {{solar luminosity|0.20|link=y}}. Its effective temperature is 4,640 K, which gives the star an orange color typical of K-type stars. Its metallicity—the proportion of elements other than hydrogen and helium—is approximately equal to the Sun's.
This star is moderately active, as shown by its spectral activity indicators and photometric data. These measurements indicate a rotation period of around 30 to 40 days, with a most likely value of 34 days. Stellar activity also creates radial velocity variations, which complicates the measurement of the mass of the planets in the system.
A companion to HD 21749 is listed in double star catalogues, a 9th-magnitude star separated by {{val|22|ul="}} in 2015, although decreasing rapidly due to the high proper motion of the primary. The companion is much more distant than the primary and the two are unrelated except being coincidentally in the same line of sight.
Planetary system
In January 2019, the discovery of an exoplanet around HD 21749 was published. The planet was identified from a single transit event detected by the TESS spacecraft, using data from the first two observation sectors of the mission. Since a single transit is insufficient to determine the orbit of a planet, astronomers used archival radial velocity data from the HARPS spectrograph to detect the planet's signal, which allowed the determination of its orbital period and mass. In April 2019, with two additional months of data from the TESS spacecraft, the orbital period of the planet was confirmed with the observation of new transits, and a second planet was discovered.
=HD 21749 c=
The inner planet, HD 21749 c (the second in order of discovery), is orbiting the star at a distance of 0.08 AU with a period of just 7.8 days. A terrestrial planet, it has a radius of {{val|1.1|ul=R+}} and was the first Earth-sized planet found by TESS. Its mass is too low to be calculated with current radial velocity data, with an upper limit of {{val|3.5|ul=M+}}; a probabilistic model estimates it is most likely between 1 and {{val|2|u=M+}}.
=HD 21749 b=
The outer planet, HD 21749 b, orbits the star at a distance of 0.21 AU with a period of 35.6 days. With a mass of {{val|20|u=M+}} and a radius of {{val|2.9|u=R+}}, it is similar to Neptune but much denser. Its density of 4.7 g/cm³ suggests it is composed of a substantial rocky core, with a radius of approximately {{val|2.1|u=R+}}, plus a relatively thick gaseous layer.
{{OrbitboxPlanet begin
| name = HD 21749
}}
{{OrbitboxPlanet
| exoplanet = c
| mass_earth = <3.5
| period = {{val|7.7902|0.0004|0.0006}}
| semimajor ={{val|0.076|0.008}}
| radius_earth = {{val|1.13|0.11|0.10}}
| eccentricity = 0
| inclination = {{val|89.44|0.36|0.52}}
}}
{{OrbitboxPlanet
| exoplanet = b
| mass_earth = {{val|20.0|2.7}}
| period = {{val|35.6133|0.0005|0.0006}}
| semimajor = {{val|0.209|0.022|0.021}}
| radius_earth = {{val|2.86|0.21|0.20}}
| eccentricity = {{val|0.164|0.062|0.058}}
| inclination = {{val|89.40|0.07|0.08}}
}}
{{Orbitbox end}}
References
{{reflist|refs=
{{cite simbad|title=HD 21749|access-date=8 January 2018}}
{{cite Gaia DR3|4673947174316727040}}
{{cite Gaia DR3|4673947071237511552}}
| title=XHIP: An extended hipparcos compilation
| last1=Anderson | first1=E. | last2=Francis | first2=Ch.
| journal=Astronomy Letters
| volume=38 | issue=5 | pages=331 | year=2012
| bibcode=2012AstL...38..331A | doi=10.1134/S1063773712050015
| arxiv=1108.4971 | s2cid=119257644 }}
| title=UBV(RI)CJHK observations of Hipparcos-selected nearby stars
| last1=Koen | first1=C. | last2=Kilkenny | first2=D.
| last3=van Wyk | first3=F. | last4=Marang | first4=F.
| display-authors=1 | journal=Monthly Notices of the Royal Astronomical Society
| volume=403 | issue=4 | date=April 21, 2010 | pages=1949–1968
| doi=10.1111/j.1365-2966.2009.16182.x | doi-access=free
| bibcode=2010MNRAS.403.1949K }}
| display-authors=1
| last1=Gray | first1=R. O. | last2=Corbally | first2=C. J.
| last3=Garrison | first3=R. F. | last4=McFadden | first4=M. T.
| last5=Bubar | first5=E. J. | last6=McGahee | first6=C. E.
| last7=O'Donoghue | first7=A. A. | last8=Knox | first8=E. R.
| title=Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample
| journal=The Astronomical Journal
| volume=132 | issue=1 | pages=161–170 | date=July 2006
| doi=10.1086/504637 | bibcode=2006AJ....132..161G
| arxiv=astro-ph/0603770 | s2cid=119476992 }}
}}
External links
- {{cite web |author=Staff |title=Stellar Overview Page - HD 21749 |url=https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=HD%2021749 |date=2019 |work=NASA Exoplanet Archive |accessdate=8 January 2019 }}
- {{cite news |last=Overbye |first=Dennis |authorlink=Dennis Overbye |title=Another Day, Another Exoplanet: NASA's TESS Keeps Counting More |url=https://www.nytimes.com/2019/01/07/science/exoplanets-tess-nasa.html |date=7 January 2019 |work=The New York Times |accessdate=8 January 2019 }}
- {{cite news |author=Massachusetts Institute of Technology |title=TESS discovers its first Earth-sized planet - Orbiting a nearby star, the new planet is the smallest identified so far by the TESS mission |url=https://www.eurekalert.org/pub_releases/2019-04/miot-tdi041619.php |date=16 April 2019 |work=EurekAlert! |accessdate=16 April 2019|author-link=Massachusetts Institute of Technology }}
{{Stars of Reticulum|state=collapsed}}
{{Portal bar|Astronomy|Biology}}
{{Sky|03|26|59.22|-|63|29|56.9}}
{{DEFAULTSORT:HD 21749}}
Category:Planetary transit variables
Category:Planetary systems with two confirmed planets